Table 2: Abundances for both components of V578 Mon, $\Delta \epsilon$ with respect to #201, and [X/H] relative to solar. Solar abundances are as listed in Table 3.
element $\Delta \epsilon_{\rm A}$ $\sigma$ $[X/H]_{\rm A}$ $\Delta \epsilon_B$ $\sigma$ [X/H]_B

C +0.10 0.09 -0.22 -0.01 0.12 -0.33

N -0.16 : -0.59 +0.06 0.10 -0.37

O -0.04 0.04 -0.34 -0.01 0.05 -0.31

Mg -0.11 0.07 -0.27 <+0.17 0.10 -0.09

Si -0.01 0.10 -0.24 +0.01 0.12 -0.22

**Table 2:** Abundances for both components of V578 Mon, $\Delta \epsilon$ with respect to #201, and [X/H] relative to solar. Solar abundances are as listed in Table 3.
element	$\Delta \epsilon_{\rm A}$	$\sigma$	$[X/H]_{\rm A}$	$\Delta \epsilon_B$	$\sigma$	[X/H]_B
C	+0.10	0.09	-0.22	-0.01	0.12	-0.33
N	-0.16	:	-0.59	+0.06	0.10	-0.37
O	-0.04	0.04	-0.34	-0.01	0.05	-0.31
Mg	-0.11	0.07	-0.27	<+0.17	0.10	-0.09
Si	-0.01	0.10	-0.24	+0.01	0.12	-0.22

Source LaTeX | All tables | In the text

	1 Introduction
	2 Method
	3 Component spectra
	4 Quantitative abundance analysis
	5 Discussion and conclusions
	References